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Scattered OH maser sources in the direction of W49N

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Date

2009-04

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Cambridge University Press

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Abstract

OH masers spots are observed with the VLBA at 1612, 1665 and 1667 MHz. The orientation of the ellipses resulting from scattering are all nearly aligned perpendicular to the galactic plane. These ordered orientation could be due to the galactic magnetic field.

Description

Restricted Access. Proceedings of the International Astronomical Union, IAU Symposium on Cosmic Magnetic Fields: From Planets, 2009.

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Citation

IAU Symposium, 2009, Vol.259, p95

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http://hdl.handle.net/2289/4147

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2009 International Astronomical Union.